Search results 19 matches in 0.002 seconds
Showing 1 - 19

1) ACE CRIS L2 1-day Z=3-28 flux data maxmize
Resource ID:spase://VSPO/NumericalData/ACE/CRIS/PT86400S
Start:1997-08-14 00:00:00 Observatory:ACE Cadence:86400 seconds
Stop:2016-09-14 08:00:05 Instrument:Cosmic Ray Isotope Spectrometer (CRIS) Resource:NumericalData
ACE CRIS L2 1-day Z=3-28 flux data at ASC

2) ACE SIS 1-Hr Key Parameter Data maxmize
Resource ID:spase://VSPO/NumericalData/ACE/SIS/PT3600S
Start:1997-08-28 00:00:00 Observatory:ACE Cadence:3600 seconds
Stop:2016-09-14 08:00:05 Instrument:Solar Isotope Spectrometer (SIS) Resource:NumericalData
ACE SIS (Solar Isotope Spectrometer) 1-Hr Key Parameter Data

3) CNOFS CINDI IVM 500 ms Ion Drift Data maxmize
Resource ID:spase://VSPO/NumericalData/CNOFS/CINDI/IVM/PT0.5S
Start:2008-08-01 00:00:00 Observatory:Communication/Navigation Outage Forecasting System (C/NOFS) Cadence:0.5 seconds
Stop:2016-09-14 07:59:51 Instrument:Coupled Ion-Neutral Dynamics Investigation (CINDI) Resource:NumericalData
This data set contains plasma parameters of the equatorial F-region in the ionosphere measured by the Ion Velocity Meter (IVM) of the Coupled Ion-Neutral Dynamics Investigation (CINDI) payload on board the CNOFS spacecraft. Data are available in HDF format, with an IDL program to read and plot them. Each file contains data from one day of spacecraft operation and the file contains eight primary geophysical parameters: the ion temperature (Ti) in degrees Kelvin, the ion flow in m/s in the ram (i.e.--spacecraft velocity) direction (+Vx in the direction of spacecraft velocity), the ion flows in m/s in the horizontal and vertical directions (Vy and Vz) at right angles to the ram direction (+Vz is downward, +Vy is roughly southward), the total ion density (Ni) (the sum of O+ and H+ and He+ concentrations) in ions/cc, and the individual H+, He+, and O+ concentrations in ions/cc. In addition, ion velocities also are given in the coordinate system of the local magnetic field (parallel, perpendicular, and meridional) in the plots and as ASCII data on the UT Dallas website. Based on the IGRF model, the data are transformed into magnetic coordinates only if all three ion velocities in the spacecraft coordinates are available and good.

4) Russian MSU Granat Heliopsheric Energetic Particles Low Noise maxmize
Resource ID:spase://VSPO/NumericalData/Granat/KS-18-M/Heliospheric/LowNoise/PT1200S
Start:1990-01-01 00:00:00 Observatory:Granat Cadence:1200 seconds
Stop:1993-12-31 23:59:59 Instrument:Energetic Particle Detectors from KS-18-M Resource:NumericalData
This set of heliospheric data in ASCII contains low noise measurements of energetic particles by the KS-18-M instrument onboard the high-altitude satellite GRANAT at large distances from the Earth. Besides the geographic coordinates of the spacecraft, the altitude is also plotted for 1989-95 as an illustration of evolution of the GRANAT's perigee. There are only several files in their extra-rectified variant.

5) Russian MSU Granat Heliopsheric Data maxmize
Resource ID:spase://VSPO/NumericalData/Granat/KS-18-M/Heliospheric/PT1200S
Start:1989-12-02 00:00:00 Observatory:Granat Cadence:1200 seconds
Stop:1995-12-16 23:59:59 Instrument:Energetic Particle Detectors from KS-18-M Resource:NumericalData
This set of heliospheric data in ASCII contains measurements of energetic particles by the KS-18-M instrument onboard the high-altitude satellite GRANAT at large distances from the Earth. Besides the geographic coordinates of the spacecraft, the altitude is also plotted for 1989-95 as an illustration of evolution of the GRANAT's perigee.

6) Russian MSU Granat Magnetospheric Particles maxmize
Resource ID:spase://VSPO/NumericalData/Granat/KS-18-M/Mag/PT1200S
Start:1989-12-05 00:00:00 Observatory:Granat Cadence:1200 seconds
Stop:1994-02-19 23:59:59 Instrument:Energetic Particle Detectors from KS-18-M Resource:NumericalData
This set of magnetospheric data contains measurements of particles by the KS-19-M instrument onboard the high-altitude satellite GRANAT during its passages through Earth's radiation belts. It also contains geographic and geomagnetic coordinates of the spacecraft. The data are in ASCII and the overview plots for several passages through the radiation belts are in gif. The altitude of the spacecraft is also plotted for 1989-95 as an illustration of evolution of the GRANAT's perigee.

7) NOAA 10 SEM MEPED Data Archive maxmize
Resource ID:spase://VSPO/NumericalData/NOAA/10/SEM/PT60S
Start:1986-10-11 00:00:00 Observatory:NOAA 10 Cadence:60 seconds
Stop:1991-08-31 23:59:59 Instrument:NOAA 10 Space Environmental Monitor Resource:NumericalData
This is the re-processed version of the MEPED (Medium Energy Proton Electron Detector) data archive from the TIROS/NOAA spacecraft containing particle count rates, fluxes, and model fields. The raw data from the NOAA archive have been processed to 1-minute resolution; magnetic field parameters (GSM Bx, By, Bz, B/Bmin, and L) are derived in 4 magnetic field models: IGRF, Tsyganenko 89 (T89), Tsyganenko 96 (T96), Tsyganenko 01 (T01); T89, T96, and T01 magnetic field models are driven with solar wind parameters and geomagnetic indices obtained from OMNI-2 data detector counts, omni and perpendicular electron and proton flux are archived.

8) STEREO-A IMPACT/LET 1-min Level 1 Ion Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/STEREO-A/IMPACT/LET/L1/PT1M
Start:2006-11-14 00:00:00 Observatory:STEREO A Cadence:1 minute
Stop:2016-09-14 07:55:45 Instrument:STEREO-A IMPACT Low Energy Telescope Resource:NumericalData
The IMPACT Low Energy Telescope (LET) data consist of 1-min resolution unsectored fluxes and counts for each of 15 single-Z ionic species at each of a species-dependent number of energy bins ranging between 9 and 16, plus 16-sectored fluxes and counts for 5 ionic species or Z groups in one (H) or two (He4, CNO, NiMgSi, Fe) energy ranges. There is much fill data. (

9) STEREO-A IMPACT/SEPT 1-min Level 1 Electron and Proton Spectra maxmize
Resource ID:spase://VEPO/NumericalData/STEREO-A/IMPACT/SEPT/L1/PT1M
Start:2006-11-14 00:00:00 Observatory:STEREO A Cadence:1 minute
Stop:2016-09-14 07:55:45 Instrument:STEREO-A IMPACT SEPT Resource:NumericalData
The IMPACT Solar Electron Proton Telescope (SEPT) Level 1 data consist of electron and proton fluxes from each of 32 energy bands that span ~20 keV to 2000(electrons) or 7000(protons) keV. These spectra are determined each minute, in each of 4 directions with 60 deg fields of view (parallel and anti-parallel to the Parker magnetic field direction, and northward and southward from the ecliptic plane.

10) STEREO-A IMPACT/SWEA 2-sec 3D Busrt Mode Distributions maxmize
Resource ID:spase://VSPO/NumericalData/STEREO-A/IMPACT/SWEA/PT2S
Start:2006-10-28 00:00:00 Observatory:STEREO A Cadence:2 seconds
Stop:2016-09-14 07:59:52 Instrument:STEREO-A IMPACT/SWEA Resource:NumericalData
This set of data comes from the IMPACT/SWEA instrument on the STEREO Ahead spacecraft. It contains 3D counts of low energy electrons distribution over a wide range of energies, angles and fluxes.

11) STEREO-A IMPACT/SWEA 30-sec 3D Distributions maxmize
Resource ID:spase://VSPO/NumericalData/STEREO-A/IMPACT/SWEA/PT30S
Start:2006-10-28 00:00:00 Observatory:STEREO A Cadence:30 seconds
Stop:2016-09-14 07:59:52 Instrument:STEREO-A IMPACT/SWEA Resource:NumericalData
This set of data comes from the IMPACT/SWEA instrument on the STEREO Ahead spacecraft. It contains 3D counts of low energy electrons distribution over a wide range of energies, angles and fluxes.

12) STEREO-B IMPACT HET Level 1 Data maxmize
Resource ID:spase://VSPO/NumericalData/STEREO-B/IMPACT/HET/L1/PT1M
Start:2006-12-01 00:00:00 Observatory:STEREO B Cadence:1 minute
Stop:2016-09-14 07:59:51 Instrument:STEREO-B IMPACT High Energy Telescope Resource:NumericalData
This data set contains Level 1 1-min data from the High Energy Telescopes (HET) of STEREO IMAPCT. Electron flux in particles/(cm2-sr-sec-MeV) are measured in 3 energy ranges: 0.7-1.4, 1.4-2.8 and 2.8-4.0 MeV. Proton flux are measured in 11 energy ranges: 13.6-15.1, 14.9-17.1, 17.0-19.3, 20.8-23.8, 23.8-26.4, 26.3-29.7, 29.5-33.4, 33.4-35.8, 35.5-40.5, 40.0-60.0, and 60.0-100.0 MeV.

13) STEREO-B IMPACT/LET 1-min Level 1 Ion Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/STEREO-B/IMPACT/LET/L1/PT1M
Start:2006-11-14 00:00:00 Observatory:STEREO B Cadence:1 minute
Stop:2016-09-14 07:55:40 Instrument:STEREO-B IMPACT Low Energy Telescope Resource:NumericalData
The IMPACT Low Energy Telescope (LET) data consist of 1-min resolution unsectored fluxes and counts for each of 15 single-Z ionic species at each of a species-dependent number of energy bins ranging between 9 and 16, plus 16-sectored fluxes and counts for 5 ionic species or Z groups in one (H) or two (He4, CNO, NiMgSi, Fe) energy ranges. There is much fill data. (

14) STEREO-B IMPACT/SEPT 1-min Level 1 Electron and Proton Spectra maxmize
Resource ID:spase://VEPO/NumericalData/STEREO-B/IMPACT/SEPT/L1/PT1M
Start:2006-11-13 00:00:00 Observatory:STEREO B Cadence:1 minute
Stop:2016-09-14 07:55:40 Instrument:STEREO-B IMPACT SEPT Resource:NumericalData
The IMPACT Solar Electron Proton Telescope (SEPT) Level 1 data consist of electron and proton fluxes from each of 32 energy bands that span ~20 keV to 2000(electrons) or 7000(protons) keV. These spectra are determined each minute, in each of 4 directions with 60 deg fields of view (parallel and anti-parallel to the Parker magnetic field direction, and northward and southward from the ecliptic plane.

15) STEREO-B IMPACT/SWEA 2-sec 3D Burst Mode Distributions maxmize
Resource ID:spase://VSPO/NumericalData/STEREO-B/IMPACT/SWEA/PT2S
Start:2006-10-28 00:00:00 Observatory:STEREO B Cadence:2 seconds
Stop:2016-09-14 07:59:51 Instrument:STEREO-B IMPACT/SWEA Resource:NumericalData
This set of data comes from the IMPACT/SWEA instrument on the STEREO Behind spacecraft. It contains 3D counts of low energy electrons distribution over a wide range of energies, angles and fluxes.

16) STEREO-B IMPACT/SWEA 30-sec 3D Distributions maxmize
Resource ID:spase://VSPO/NumericalData/STEREO-B/IMPACT/SWEA/PT30S
Start:2006-10-28 00:00:00 Observatory:STEREO B Cadence:30 seconds
Stop:2016-09-14 07:59:51 Instrument:STEREO-B IMPACT/SWEA Resource:NumericalData
This set of data comes from the IMPACT/SWEA instrument on the STEREO Behind spacecraft. It contains 3D counts of low energy electrons distribution over a wide range of energies, angles and fluxes.

17) Ulysses GAS UV Full-Sky Data maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/GAS/Full-Sky/PT24H
Start:1990-10-27 00:00:00 Observatory:Ulysses Cadence:24 hours
Stop:2007-08-18 23:59:59 Instrument:Ulysses Interstellar Neutral Gas (GAS) Experiment Resource:NumericalData
This Ulysses GAS experiment data set consists of pixel map data and image files for sky maps generated from GAS measurements in a mode primarily sensitive to ultraviolet photons. The accumulated counts and Ecliptic (spacecraft-centered) angle coordinates for each sky map pixel are given in the ascii files *.TXT. The positions of the Sun and the planets vary with time and with the position of the spacecraft along its trajectory, while the positions of stars remain fixed. The full images are provided in GIF (*.GIF files) and postscript (*.PS files) format, the GIF files being easily viewed on-line (see below) with an Internet web browser. The actual positions of Sun, Earth, and Jupiter are indicated by yellow, green, and white dots, respectively. The area around the Sun is excluded from observation to avoid damaging intensities from direct sunlight. The files USER_GUIDE.TXT, FORMAT.TXT, and REFERENCE.TXT, respectively, give an overall description of the various datatypes, the record format for the DATA datatype, and a list of GAS-related publications. The users guide defines the nomenclature of the file names.

18) Ulysses GAS Interstellar Helium Maps maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/GAS/Interstellar-Helium/PT24H
Start:1990-10-27 00:00:00 Observatory:Ulysses Cadence:24 hours
Stop:2007-11-25 23:59:59 Instrument:Ulysses Interstellar Neutral Gas (GAS) Experiment Resource:NumericalData
This Ulysses GAS experiment data set consists of pixel map data and image files for sky maps generated from GAS measurements in the mode primarily sensitive to neutral helium atoms from inflow of interstellar gas into the heliosphere. The accumulated counts and Ecliptic (spacecraft-centered) angle coordinates for each sky map pixel are given in the ascii files *.TXT. The positions of the Sun and the planets vary with time and with the position of the spacecraft along its trajectory, while the positions of stars remain fixed. The full images are provided in GIF (*.GIF files) and postscript (*.PS files) format, the GIF files being easily viewed on-line (see below) with an Internet web browser. The actual positions of Sun, Earth, and Jupiter are indicated by yellow, green and white dots, respectively. The area around the Sun is excluded from observation to avoid damaging intensities from direct sunlight. The files USER_GUIDE.TXT, FORMAT.TXT, and REFERENCE.TXT, respectively, give an overall description of the various datatypes, the record format for the DATA datatype, and a list of GAS-related publications. The users guide defines the nomenclature of the file names. Further details about the data and the experiment may be found in Witte et al., Astron. Astrophys. Suppl. Ser., 92, No. 2, 333-348, 1992 (NSSDC TRF # B40459-000A). Data analysis methods for interstellar helium are described in Banaszkiewicz et al., Astron. Astrophys. Suppl. Ser., 120, 587-602, 1996 (B45706-000A).

19) Russian MSU Zond-3 Heliopsheric Data maxmize
Resource ID:spase://VSPO/NumericalData/Zond-3/KS-18/Heliospheric/PT4H
Start:1965-07-19 00:00:00 Observatory:Zond 3 Cadence:4 hours
Stop:1966-01-21 23:59:59 Instrument:Energetic Particles, MSU-TASPD Resource:NumericalData
This set of heliospheric data in ASCII contains measurements of energetic particles by the KS-18 instrument onboard the third Russian space probe of the Zond series at heliocentric distances larger than 1 AU. It includes proton flux intensities at >30 MeV energy from Sun (gas-discharge counter) and at 1-5 MeV energy arriving from the direction perpendicular to the Sun-spacecraft line (stand-alone SSD sensor of 35 micron Si). Subdirectory /lownoise contains the same measured data but in its extra-rectified variant. Besides the trajectory data in two coordinate systesms, there are overview plots in GIF.

Showing 1 - 19